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Paolo Privitera has been awarded an Advanced Grant by the European Research Council
April 9, 2018
4 M$ Advanced Grant by the European Research Council to search for light dark matter particles with DAMIC. The DArk Matter In CCDs experiment (DAMIC) is designed to detect the tiny signals produced by the interaction of dark matter with the bulk silicon of ~mm-thick charge-coupled devices. The kg-size DAMIC detector to be installed at the Laboratoire Souterrain de Modane in France will search for low-mass dark matter particles with unprecedented sensitivity. The European Research Council "selects and funds the very best, creative researchers of any nationality to run projects based in Europe", with Principal Investigators of Advanced Grants identified as "exceptional leaders in terms of originality and significance of their research contributions."
Congratulations to Nora Shipp!
April 5, 2018
SCGSR Fellowship and a URA Visiting Scholars Program award to work with Fermilab scientists on using stellar streams to learn about dark matter in the Milky Way.
"Nora Shipp has carried out an analysis of the wide-field distribution of stars in the Dark Energy Survey (DES) footprint on the sky and identified several known stellar streams and discovered new streams. Stellar streams are an "archeological" record of the accretion history of the Milky Way and can be used as probes of properties of dark matter and of the Milky Way gravitational potential.
This project resulted in a paper that presented one of the most spectacular scientific results of the first year DES data and the results were a subject of a number of press releases and were widely covered in the media. In collaboration with DES scientists at Fermilab, Nora is continuing to characterize the streams analyzed in the DES and is planning to search for gaps in the streams and to model them using techniques developed by a former KICP student, Denis Erkal, as part of his postdoc work with Vasily Belokurov at Cambridge. Nora also plans to carry out N-body simulations for more detailed modeling of the streams. This program can potentially provide a new and unique probe of existence of dark matter clumps of mass $approx 10^6-10^7$ solar masses in the Milky Way, thereby constraining properties of dark matter itself, and to constrain properties of the Milky Way potential itself. DoE and URA fellowships that Nora received will help to carry out the first stages of this longer term PhD thesis program."
- Andrey Kravtsov, scientific advisor
Katrina Miller won a 2018 NSF Graduate Research Fellowship
April 3, 2018
Katrina is a member of the XENON collaboration, an international research group operating a 3.3-ton liquid xenon detector in search for dark matter. Her current project focuses on characterizing processes that produce single electron events in our detector as a source of low-energy background that would mask potential dark matter signals interacting via electronic, rather than nuclear, recoil.
The NSF Graduate Research Fellowship Program (GRFP) has announced the offer of 2,000 fellowship awards, following a national competition. The program recruits high-potential, early-career scientists and engineers and supports their graduate research training in science, technology, engineering and mathematics (STEM) fields.
Kaeli Hughes won a 2018 NSF Graduate Research Fellowship
April 3, 2018
"Dear Kaeli Hughes:
I am pleased to inform you that you have been selected to receive a 2018 National Science Foundation (NSF) Graduate Research Fellowship Program (GRFP) Fellowship. Your selection was based on your demonstrated potential to contribute to strengthening the vitality of the U.S. science and engineering enterprise. Your selection as an NSF Graduate Fellowship awardee is a significant accomplishment. We wish you success in your graduate studies in science, technology, engineering, and mathematics (STEM) or in STEM education, and continued success in achieving your career aspirations. We look forward to learning about your achievements and contributions during your graduate study and beyond.
Division of Graduate Education"
PFC Director Michael Turner presented the 2018 Oppenheimer Lecture at the University of California at Berkeley
March 6, 2018
Big ideas like the deep connections between quarks and the cosmos and powerful instruments like the Hubble Space Telescope and Large Hadron Collider have advanced our understanding of the universe. We can now trace its history from the big-bang beginning 13.8 billion years ago through an early state of quantum fluctuations to a soup of quarks and other particles, from the formation of nuclei and atoms to the emergence of stars and galaxies, and finally to its expansion today. This lecture describes what we know, what we are trying to figure out and the excitement of the adventure.
Joshua Frieman will become the Head of Particle Physics Division at Fermilab
February 19, 2018
Congratulations to Abigail Vieregg and Eduardo Rozo!
February 14, 2018
2018 Cottrell Scholars given to outstanding early career academic scientists. The designation comes with a $100,000 award for each recipient for research and teaching.
"The Cottrell Scholar (CS) program champions the very best early career teacher-scholars in chemistry, physics and astronomy by providing these significant discretionary awards," said RCSA President and CEO Daniel Linzer.
Cottrell Scholars engage in an annual networking event, providing them an opportunity to share insights and expertise through the Cottrell Scholar Collaborative. This year’s Cottrell Scholar Conference will be held July 11-13 in Tucson, Ariz., and is expected to draw about 100 top educators from around the U.S.
Congratulations to Dan Scolnic!
November 8, 2017
U.S. National Academies of Sciences, Engineering, and Medicine.
Congratulations to Eric Dahl!
November 2, 2017
Citation: "for fundamental contributions to the development of new techniques for the direct detection of dark matter, including the bubble chamber and xenon time projection chamber."
Henry Primakoff Award for Early-Career Particle Physics
To recognize outstanding contributions made by physicists who are just beginning their careers, and to help promote the careers of exceptionally promising young physicists. The prize is given annually and will consist of $1,500 and a certificate citing the contributions of the recipient, plus an allowance for travel to an APS meeting to receive the award and deliver an invited lecture.Learn more >>
Gravitational Waves Events
October 13, 2017
FIRST, On Monday, October 16th at 09:00 CDT, the National Science Foundation will host a press briefing at the National Press Club in Washington, D.C., bringing together scientists from the Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo collaborations, as well as representatives from some 70 observatories. This will be live-streamed and we will set up a live viewing with some of the involved University of Chicago scientists in the lobby of ERC, as well as in room 201 of the Physics Research Center.
The press briefing will begin with an overview of new findings from LIGO, Virgo and partners that span the globe, followed by details from telescopes that work with the LIGO and Virgo collaborations to study extreme events in the cosmos.
The discovery of gravitational-waves by LIGO opened a new window to the Universe and involved several UChicago scientists. This year's Nobel Prize in Physics recognized three scientists for their contributions to the LIGO detector and the first observation of gravitational waves.
SECOND, there will be a special, more technical colloquium on the topic Monday, October 16th at 4:00 p.m. CDT in ERC 161, featuring University scientists Daniel Holz and Joshua Frieman, followed by discussion and comments by Holz, Frieman, Hubble Fellow Dan Scolnic, University Professor Wendy Freedman, and students and postdocs involved in the new findings. Following the discussion there will be a reception in the atrium.
THIRD, there will be an event on Tuesday, October 17th from 5:00 - 7:00 p.m. in Kersten Physics Teaching Center (KPTC 120), consisting of about 5 short presentations by graduate students and postdocs and a Q&A/discussion. This will be geared more to the general public and university undergraduates.
I encourage you to join us for any of these special gatherings.
Dean of the Physical Sciences
The University of Chicago
Congratulations to Dr. Alessandro Manzotti!
July 24, 2017
"Unveiling the early Universe: delensing the Cosmic Microwave Background with galaxy surveys".
"Alessandro led the team that carried out the first 'de-lensing' of the polarization in the cosmic microwave background. Using data from the South Pole Telescope, the team used software to undo what billions of years of propagation through the clumpy universe has done: distorted the pattern of polarization. This first demonstration is the harbinger of what will ultimately become an essential tool in analyses of future SPT CMB-Stage 4 data."
- Scott Dodelson, Ph.D. advisor
Alessandro has received a Lagrange Fellow position at the Institut d'Astrophysique de Paris.
Congratulations to Dr. Laura Mocanu!
July 21, 2017
"Measuring the cosmic microwave background gravitational lensing potential and its power spectrum with SPTpol".
"Monica has make many important contributions to the analysis of South Pole Telescope CMB data. For her thesis she has used SPTpol temperature and polarization data to produce the most sensitive CMB lensing reconstruction of the mass distribution in the universe, paving the wave for SPT-BICEP B-mode delensing and other cosmological analysis."
- John Carlstrom, Ph.D. advisor
Laura has received a Postoctoral fellowship at the University of Oslo.
John Carlstrom becomes the new Chair of the Department of Astronomy & Astrophysics
July 13, 2017
Effective October 1, 2017, John Carlstrom will become the Chair of Astronomy and Astrophysics. His scientific excellence will serve the department well in the coming years.
I thank Angela Olinto for her excellent service as Chair of Astronomy and Astrophysics.
I look forward to working closely with John as he takes on leadership of the Department. Please join me in congratulating him on this appointment.
Dean of the Physical Sciences Division
Congratulations to Dr. Chen He Heinrich!
June 19, 2017
"Lensing Bias to CMB Polarization Measurements of Compensated Isocurvature Perturbations".
Chen has received a postdoc position in cosmology at the Jet Propulsion Laboratory, NASA.
Space Explorers Program Evaluation and Experiments Featured at the 2017 National Science Teachers Association (NSTA) Meeting Los Angeles, CA
June 14, 2017
Randall H. Landsberg presented "Space Explorers: 25 Years of Inner-city Students Out of School Time Explorations" as part of the "mission possible" thread at the NSTA national conference. The talk included data on how students in the program are out preforming their peers and exemplar, hands-on, inquiry based experiments. The experiments both involved measurements but in very different realms: the size of the universe and the response rates of rods compared to cones in the human eye.
Space Explorers Compared to Chicago Public Schools.
Undergraduate First-Year STEM Majors National Data Comparison.
Since 1991 Space Explorers has offered first generation, low income inner-city students and university astrophysics researchers the opportunity to explore together (with over one hundred contact hours a year). An external evaluation probed the impacts of this program on the hundreds of students and instructors involved. We will examine the evaluation findings, which map well to the recent NRC study on out of school time programs. We will also explore some of our favorite lab activities, hear about taking students to Yerkes Observatory for residential science institutes, and discuss best practices for university and community based organization partnerships. Take home new ideas for student labs and partnerships.
Space Explorers Careers
(respondent 4 years past high school graduation n~100).
Congratulations to Dr. Hsin-Yu Chen!
June 12, 2017
"Multi-messenger Astronomy with Advanced LIGO-Virgo".
"Hsin-Yu's work is helping set the stage for the new era of gravitational-wave astronomy. She has played an active role within the LIGO collaboration in the analysis of our first detections, while also becoming a leader in the field of multi-messenger astronomy."
- Daniel E. Holz, PhD advisor
Hsin-Yu has received a postdoc position at the Black Hole Initiative (Harvard).
Congratulations to Dr. Michael Fedderke!
June 9, 2017
"Studies in Higgs physics, particle dark matter and early universe".
"Michael's thesis work covers several important aspects of particle physics and cosmology. It includes detailed studies on the signal of dark matter annihilation in the galactic halo. After producing an interesting paper on the heavy particle production in the early universe, he delved into Higgs physics. He evaluated the potential of discovering new physics via fermionic Higgs portal, which has implications for the physics reach of both current and future colliders. In his most recent project, he has also constructed a model which addressed the little hierarchy problem in the composite Higgs scenario using cosmological evolution of an axion like field."
- LianTao Wang, PhD advisor
Michael has received a joint postdoc position at Stanford University and UC Berkeley.
Congratulations to PFC member Wayne Hu, newly inducted NAS member!
May 1, 2017
Members are elected to the National Academy of Sciences in recognition of their distinguished and continuing achievements in original research.
Video of the Presentation Ceremony
Congratulations to PFC member Joshua Frieman!
April 27, 2017
The Division of Astrophysics (DAP), organized in 1970, engages in observational and theoretical investigation that relates to the study of physical processes in stars and other discrete galactic sources, galactic structure and evolution, the early history and evolution of the Universe, and the Sun and solar activity. Division interests also have significant overlap with other APS divisions such as Particles and Fields, Nuclear Physics, and Plasma Physics.
The Halo Boundary of Galaxy Clusters in SDSS
April 24, 2017
recent study, which presents strong evidence for the physical edge of galaxy clusters using public data from the Sloan Digital Sky Survey.
The existence of such physical edges associated with sharp density drops due to the density caustics formed by accreting matter was predicted by KICP researchers Benedikt Diemer and Andrey Kravtsov in 2014, as part of Diemers PhD research. In a follow-up study, Diemer, Kravtsov and a former KICP fellow Surhud More (currently at Institute of Physics of the Universe, Tokyo, Japan) have shown that the-edges can be considered to be natural physical boundary of dark matter halos that provide the gravitational "back-bone" for the structures observed in the galaxy distribution.
In the recent study, co-led by Chihway Chang and Eric Baxter - a former KICP student and currently a postdoctoral fellow at the University of Pennsylvania - the density drop associated with the halo edges was detected in the galaxy distribution around cluster centers.
Cosmological simulations show that massive galaxy clusters we see today have been accreting galaxies into their deep gravitational potential over the cosmic time. The process of galaxies "falling into" the cluster's potential well is a fairly clean and universal process that depends only on basic quantities of the cluster such as mass and accretion rate. One of the result of this simple picture is a sharp feature in the number density of galaxies around clusters - an imprint of the caustic formed by the infalling galaxies as they reach the first apocenter of their orbit, or the "edge" of the galaxy cluster. Researchers called the distance of the edge the "splashback" radius, as galaxies literally "splashing back" to that radius after they accrete onto cluster.
Together with collaborators in UPenn and UIUC, that included KICP faculty Andrey Kravtsov, Chihway Chang and Eric Baxter, examined distribution of galaxies around a sample of clusters identified within the SDSS. The existence of the edge in the galaxy distribution within clusters was confirmed. In addition, the analysis revealed that properties of galaxies around cluster are sensitive to existence of the edge. Outside the splashback radius, the mix of red and blue galaxies was approximately independent of the distance from the cluster center, while inside the splashback radius the mix is abruptly changes towards a larger fraction of red galaxies. This indicates that the edge is a real dynamical feature and that majority of galaxies get transformed by the cluster environment from blue to red in less than one orbital period.
This figure shows the fraction of red and blue galaxies around galaxy clusters. The sharp change in the red fraction indicates that galaxy tend to turn red once they enter the edge of the cluster, which is marked by the grey vertical band. (Figure modified from the paper "The Halo Boundary of Galaxy Clusters in the SDSS".)
Related KICP references: